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Class 10 · Science · Physics

Chapter 9: Light – Reflection and Refraction

Revision notes, practice numericals, a question bank, assertion and reason questions and answers to the NCERT questions. Tap a group to open it; opening one closes the others.

9.1Reflection of lightLaws, plane mirror images

What is reflection?

When light falls on a polished surface such as a mirror, it bounces back into the same medium. This is reflection. Light seems to travel in straight lines, and reflecting surfaces of all kinds obey the laws of reflection.

Laws of reflection

  • The angle of incidence is equal to the angle of reflection: ∠i = ∠r.
  • The incident ray, the normal to the mirror at the point of incidence and the reflected ray all lie in the same plane.
NormalIncident rayReflected rayirPoint of incidence∠i = ∠r, and the incident ray, normal and reflected ray lie in one plane.
Laws of reflection.

Image in a plane mirror

  • The image is virtual and erect.
  • It is the same size as the object (magnification +1).
  • It is formed as far behind the mirror as the object is in front.
  • It is laterally inverted (left appears as right).
9.1.1Spherical mirrorsConcave, convex and their terms

Types

A spherical mirror is part of a hollow sphere. If the inner surface is the reflecting surface, it is a concave mirror; if the outer surface reflects, it is a convex mirror.

Important terms

  • Pole (P): the centre of the reflecting surface.
  • Centre of curvature (C): the centre of the sphere of which the mirror is a part.
  • Radius of curvature (R): the radius of that sphere, equal to the distance PC.
  • Principal axis: the straight line through P and C.
  • Aperture: the diameter of the reflecting surface.
  • Principal focus (F): the point on the principal axis where rays parallel to the axis meet (concave) or appear to come from (convex) after reflection.
  • Focal length (f): the distance PF.

Relation between f and R

For spherical mirrors of small aperture, the principal focus lies midway between the pole and the centre of curvature.

R = 2f    or    f = R / 2
9.1.2Ray diagrams for mirrorsRules and images formed

Three rules for drawing rays

  • A ray parallel to the principal axis passes through the principal focus (concave) or appears to diverge from it (convex) after reflection.
  • A ray passing through the principal focus (concave) becomes parallel to the principal axis after reflection.
  • A ray through the centre of curvature is reflected back along the same path, since it strikes the mirror along the normal.

Concave mirror: object beyond C

The image is formed between F and C. It is real, inverted and diminished.

PFCOI
Concave mirror, object beyond C: real, inverted, diminished image between F and C.

Concave mirror: object between P and F

The image is formed behind the mirror. It is virtual, erect and enlarged. This is how a shaving mirror works.

PFCOI
Concave mirror, object between P and F: virtual, erect and enlarged image behind the mirror (dashed lines are extensions).

Images formed by a concave mirror

Object positionImage positionSizeNature
At infinityAt FHighly diminished, point-sizedReal and inverted
Beyond CBetween F and CDiminishedReal and inverted
At CAt CSame sizeReal and inverted
Between C and FBeyond CEnlargedReal and inverted
At FAt infinityHighly enlargedReal and inverted
Between P and FBehind the mirrorEnlargedVirtual and erect

Convex mirror

For every position of the object, a convex mirror forms a virtual, erect and diminished image behind the mirror, between P and F. For an object at infinity the image is at F and highly diminished.

PFOI
Convex mirror: virtual, erect and diminished image behind the mirror, whatever the object distance.
9.1.3Uses of mirrorsWhere each type is used

Concave mirrors

  • In torches, searchlights and vehicle headlights, to get a powerful parallel beam of light (the bulb is at the focus).
  • As shaving mirrors, to see a larger, erect image of the face.
  • By dentists, to see a large image of the teeth.
  • In solar furnaces, to concentrate sunlight at the focus.

Convex mirrors

Used as rear-view (wing) mirrors in vehicles. They always give an erect, diminished image, and they have a much wider field of view than a plane mirror, so the driver can see traffic far behind.

9.1.4Sign convention, mirror formulaNew Cartesian sign convention

New Cartesian sign convention

  • The object is always placed to the left of the mirror, so light falls from the left.
  • All distances parallel to the principal axis are measured from the pole.
  • Distances to the right of the pole (along +x) are positive; to the left (−x) are negative.
  • Distances above the principal axis (+y) are positive; below (−y) are negative.

So the object distance u is always negative. For a concave mirror f is negative; for a convex mirror f is positive.

Mirror formula

The relation between object distance u, image distance v and focal length f is

1/v + 1/u = 1/f

Magnification

Magnification m is the ratio of the height of the image (h') to the height of the object (h). It is also related to distances:

m = h'/h = −v/u
  • m is negative for a real, inverted image; positive for a virtual, erect image.
  • |m| > 1: enlarged; |m| < 1: diminished; |m| = 1: same size.
9.2Refraction of lightBending of light between media

What is refraction?

When light travels obliquely from one transparent medium to another, its direction changes at the boundary. This is refraction. It happens because the speed of light is different in different media.

Rarer and denser

  • Rarer to denser medium (air to glass): the ray bends towards the normal.
  • Denser to rarer medium (glass to air): the ray bends away from the normal.
  • A ray travelling along the normal does not bend.
Air (rarer)Glass (denser)irIncident rayRefracted rayRarer → denser: bends towards the normal (r < i). Denser → rarer: bends away.
Refraction at an air-glass surface.

Glass slab

In a rectangular glass slab, refraction takes place at both the air-glass and glass-air faces. The emergent ray is parallel to the incident ray but is laterally shifted.

Incident rayEmergent rayGlass slabThe emergent ray is parallel to the incident ray, only shifted sideways.
Refraction through a rectangular glass slab.

Laws of refraction

  • The incident ray, the refracted ray and the normal lie in the same plane.
  • Snell's law: for a given pair of media and a given colour of light, sin i / sin r = constant.

Refractive index

The refractive index of a medium (with respect to vacuum) is the ratio of the speed of light in vacuum to its speed in that medium.

n = c / v

Light travels at 3 × 10⁸ m/s in vacuum. A medium with a greater refractive index is optically denser and light travels more slowly in it. For example, n for water is 1.33, glass about 1.5 and diamond 2.42.

9.2.1Spherical lensesConvex and concave lenses

Types

  • A convex lens is thicker at the centre. Parallel rays converge at a point, so it is a converging lens.
  • A concave lens is thicker at the edges. Parallel rays diverge, so it is a diverging lens.

Important terms

  • Optical centre (O): the central point of the lens; a ray through it goes straight.
  • Principal axis: the line through the two centres of curvature.
  • Principal focus (F): a lens has two foci, F₁ and F₂, one on each side.
  • Focal length (f): the distance from the optical centre to the principal focus.
  • Aperture: the effective diameter of the circular outline of the lens.

Rules for ray diagrams

  • A ray parallel to the principal axis passes through the second focus F₂ (convex) or appears to come from the first focus F₁ (concave).
  • A ray through the first focus F₁ emerges parallel to the principal axis (convex).
  • A ray through the optical centre emerges without any deviation.
9.2.2Images formed by lensesConvex and concave lens images

Convex lens: object beyond 2F₁

The image is real, inverted and diminished, between F₂ and 2F₂.

F₁F₂2F₁2F₂OObjectImage
Convex lens, object beyond 2F: real, inverted, diminished image between F and 2F.

Convex lens: object between O and F₁

The image is virtual, erect and enlarged, on the same side as the object. A convex lens used like this is a magnifying glass.

F₁F₂2F₁2F₂OObjectImage
Convex lens, object between O and F: virtual, erect, enlarged image on the same side (a magnifying glass).

Images formed by a convex lens

Object positionImage positionSizeNature
At infinityAt F₂Highly diminished, point-sizedReal and inverted
Beyond 2F₁Between F₂ and 2F₂DiminishedReal and inverted
At 2F₁At 2F₂Same sizeReal and inverted
Between F₁ and 2F₁Beyond 2F₂EnlargedReal and inverted
At F₁At infinityHighly enlargedReal and inverted
Between O and F₁Same side as objectEnlargedVirtual and erect

Concave lens

A concave lens always forms a virtual, erect and diminished image on the same side as the object. For an object at infinity the image is at F₁, highly diminished; for an object between infinity and O the image is between F₁ and O.

F₁F₂2F₁2F₂OObjectImage
Concave lens: virtual, erect and diminished image between O and F on the same side as the object.
9.2.3Lens formula and powerFormula, magnification, dioptre

Lens formula

The same sign convention is used, with distances measured from the optical centre.

1/v − 1/u = 1/f

For a convex lens f is positive; for a concave lens f is negative.

Magnification

The magnification produced by a lens is the ratio of the image height to the object height.

m = h'/h = v/u

A positive m means a virtual, erect image; a negative m means a real, inverted image.

Power of a lens

The power of a lens is the reciprocal of its focal length in metres. Its SI unit is the dioptre (D): one dioptre is the power of a lens of focal length 1 metre.

P = 1 / f

A convex lens has positive power; a concave lens has negative power. Opticians use power to prescribe lenses.

Lenses in contact

The power of a combination of lenses placed in contact is the algebraic sum of their powers.

P = P₁ + P₂ + P₃ + …